Wave and stability properties of black holes

Details Wave and stability properties of black holes Wave and stability properties of black holes

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.150..189m&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 150, no. 1, Dec. 1988, p. 189-199.

Statistics

Computation

1

Black Holes (Astronomy), Computational Astrophysics, Gravitational Effects, Perturbation Theory, Wave Equations, Green'S Functions, Klein-Gordon Equation, Photons, Schwarzschild Metric

Scientific paper

The wave equation governing the gravitational perturbations of a Schwarzschild black hole has been transformed from its standard form to a Klein-Gordon-type wave equation. The present formulation shows that incoming waves below a critical frequency are completely reflected while those above it are transmitted. It is predicted that the neighborhood around which the metric is locally unstable will behave as a wave emitter.

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